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• W3101599507 abstract "The production of GWs during preheating in the Starobinsky model with a nonminimally coupled auxiliary scalar field is studied through the lattice simulation in this paper. We find that the GW spectrum $Omega_{rm gw}$ grows fast with the increase of the absolute value of coupling parameter $xi$. This is because the resonant bands become broad with the increase of $|xi|$. When $xi<0$, $Omega_{rm gw}$ begins to grow once the inflation ends and grows faster than the case of $xi>0$. $Omega_{rm gw}$ reaches the maximum at $xi=-20$ ($xi=42$ for the case $xi>0$) and then decreases with slight oscillation. Furthermore we find that the GWs produced in the era of preheating satisfy the limits from the Planck and next-generation CMB experiments." @default.
• W3101599507 created "2020-11-23" @default.
• W3101599507 creator A5000918733 @default.
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• W3101599507 date "2020-06-01" @default.
• W3101599507 modified "2023-09-26" @default.
• W3101599507 title "Production of gravitational waves during preheating in the Starobinsky inflationary model" @default.
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• W3101599507 doi "https://doi.org/10.1140/epjc/s10052-020-8061-0" @default.
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